Newtonian gravity from Higgs condensates
| dc.creator | Consoli, M. | |
| dc.creator | Siringo, F. | |
| dc.date | 1999-10-18 | |
| dc.date | 1999-11-30 | |
| dc.date.accessioned | 2026-07-07T04:08:23Z | |
| dc.date.available | 2026-07-07T04:08:23Z | |
| dc.description | We propose a description of {\it Newtonian} gravity as a long wavelength excitation of the scalar condensate inducing electroweak symmetry breaking. Indeed, one finds a $-{{G_F}\overη}{{m_im_j}\over{r}}$ long-range potential where $G_F$ is the Fermi constant and $η\equiv {{M^2_h}\over{2m^2}} $ is determined by the ratio between the Higgs mass $M_h$ and the mass m of the elementary quanta of the symmetric phase (`phions'). The parameter $η$ would diverge in a true continuum theory so that its magnitude represents a measure of non-locality of the underlying field theory. By identifying $G\equiv {{G_F}\overη}$ with the Newton constant and assuming the range of Higgs mass $M_h \sim 10^{2}-10^{3}$ GeV one obtains $m=10^{-4}-10^{-5}$ eV and predicts typical `fifth-force' deviations below the centimeter scale. Relation to Einstein gravity and string theory is discussed. The crucial role of the first-order nature of the phase transition for the solution of the so-called `hierarchy problem' is emphasized. The possible relevance of the picture for the self-similarity of the universe and for a new approach to the problem of dark matter is discussed. | |
| dc.description | Interpretation of the gap-less mode of the Higgs field as a Goldstone boson of a spontaneously broken continuous simmetry that does not exist in the simmetric phase | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9910372 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9910372 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/49510 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.subject | Astrophysics | |
| dc.title | Newtonian gravity from Higgs condensates | |
| dc.type | text |